6 October 2005 Geant4 Workshop, Leuven, Belgium Geant4 Model of SIXS Particle Instrument and Preliminary Simulation Results Lehti, J. (ASRO) Valtonen,

Slides:



Advertisements
Similar presentations
David Rothery, Dept of Earth & Environmental Sciences X-Ray detection techniques and the BepiColombo-MIXS instrument.
Advertisements

The BepiColombo Mission
Ion Beam Analysis techniques:
Simulation of X-ray Fluorescence and Application to Planetary Astrophysics A. Mantero, M. Bavdaz, A. Owens, A. Peacock, M. G. Pia IEEE NSS -- Portland,
Analysis of Mercury’s X-ray fluorescence M. Laurenza, M. Storini and A. Gardini IFSI-INAF, Via del Fosso del Cavaliere, 100, Rome 00133, Italy Joint SERENA.
Test Beam Simulation for ESA BepiColombo Mission Marcos Bavdaz, Alfonso Mantero, Barbara Mascialino, Petteri Nieminen, Alan Owens, Tone Peacock, Maria.
BepiColombo GW Fraser Space Research Centre, Department of Physics and Astronomy, University of Leicester, Leicester LE1 7RH 1. The BepiColombo Mission.
Simulations with ‘Realistic’ Photon Spectra Mike Jenkins Lancaster University and The Cockcroft Institute.
D E S I R E Dose Estimation by Simulation of the ISS Radiation Environment Geant4 simulations of the Columbus/ISS radiation.
GSEM project SPENVIS/GEANT4 Workshop, Leuven, Belgium, October 2005 Daniel Haas, DPNC Genève Outline Description of GSEM HEP Range Telescope Radiation.
Cross-calibration of SOHO/ERNE proton and heavy ion measurements with other particle instruments at L1 E. Valtonen, M. Paassilta, R. Vainio, O. Raukunen,
1 Update and functional test results for SWIM David McCann Solar system physics and space technology IRF, Kiruna Supervisor: Professor Stas Barabash David.
BLM review Mario Santana Leitner OUTLOOK ON FLUKA SIMULATIONS FOR UDULATOR DAMAGE AND BLM RESPONSE Mario Santana Leitner, Alberto.
Effects of Solar Energetic Particle Events on the Martian Surface and Atmosphere F Leblanc, DA Brain, JG Luhmann, GT Delory, RA Mewaldt, CM Cohen 2004.
Geant4 Application for Japanese Space Science Missions from 2006 to Future Masanobu Ozaki (ISAS/JAXA and JST/CREST)
GEANT4 simulations for the Lund R 3 B prototype Douglas Di Julio Lund University, Lund, Sweden.
Instrumental effects on HED anisotropy measurements Oskari Saloniemi, SRL workshop
etc… Analysing samples with complex geometries Particles Inclusions
experimental platform
The Time-of-Flight system of the PAMELA experiment: in-flight performances. Rita Carbone INFN and University of Napoli RICAP ’07, Rome,
Workshop on Physics on Nuclei at Extremes, Tokyo Institute of Technology, Institute for Nuclear Research and Nuclear Energy Bulgarian Academy.
SMRD April 2007 Status of the atmospheric muon studies Piotr Mijakowski OUTLINE: Primary muon spectrum at the sea level Primary muon.
Alfonso Mantero, INFN Genova Models for the Simulation of X-Ray Fluorescence and PIXE A. Mantero, S. Saliceti, B. Mascialino, Maria Grazia Pia INFN Genova,
ILWS and Finland Hannu Koskinen Finland and ILWS2 ILWS science in Finland Finnish Meteorological Institute, Helsinki Magnetospheres.
Space Research Centre Silicon Carbide X-Ray detectors for Planetary Exploration Dr. John E. Lees University of Leicester 8 th International Conference.
SuperNEMO Simulations Darren Price University of Manchester July, 2005.
Space Instrumentation. Definition How do we measure these particles? h p+p+ e-e- Device Signal Source.
2001 Mars Odyssey GRS RDS 1 HEND Workshop 2002 May 20 th – 22 nd 2002 Mars Odyssey Gamma-Ray Spectrometer Richard Starr NASA/GSFC – Catholic University.
Coordinated Observations between MPO and MMO Harri Laakso ESA/ESTEC, Noordwijk.
Normalisation modelling sources Geant4 tutorial Paris, 4-8 June 2007 Giovanni Santin ESA / ESTEC Rhea System SA.
Stopped Muon/Pion Measurements Jim Miller, BU May 2012 UW Test Beam Meeting.
THE FAST X-RAY MONITOR (FXM) BASED ON YAP:CE SCINTILLATOR (YTTRIUM ALUMINUM PEROVSKITE ACTIVATED BY CERIUM) FOR THE “CORONAS-PHOTON” SATELLITE PROJECT.
Susanna Guatelli & Barbara Mascialino G.A.P. Cirrone (INFN LNS), G. Cuttone (INFN LNS), S. Donadio (INFN,Genova), S. Guatelli (INFN Genova), M. Maire (LAPP),
Currently the Solar Energetic Particle Environment Models (SEPEM) system treats only protons within the interplanetary environment, and the shielding analysis.
V.Dzhordzhadze1 Nosecone Calorimeter Simulation Vasily Dzhordzhadze University of Tennessee Muon Physics and Forward Upgrades Workshop Santa Fe, June 22,
Test Beam Simulation for ESA BepiColombo Mission Marcos Bavdaz, Alfonso Mantero, Barbara Mascialino, Petteri Nieminen, Alan Owens, Tone Peacock, Maria.
IDEE, The Electron Spectrometer of the Taranis Mission J.-A. Sauvaud 1, A. Fedorov 1, P. Devoto 1, C. Jacquey 1, L. Prech 2, Z. Nemecek 2, F. Lefeuvre.
IDEE, The Electron Spectrometer for the Taranis Mission J.-A. Sauvaud 1, P. Devoto, A. Fedorov 1, G. Orttner 1, O. Chasselat 1, K. Wong 1, L. Prech 2,
Monte Carlo Simulation Study of In-orbit Background for the Soft Gamma-ray Detector onboard ASTRO-H Mizuno T., Hiragi K., Fukazawa Y., Umeki Y. (Hiroshima.
Determination of activity of 51 Cr source on gamma radiation measurements V.V.Gorbachev, V.N.Gavrin, T.V.Ibragimova, A.V.Kalikhov, Yu.M.Malyshkin,A.A.Shikhin.
2 Jun 2022 Jan 2030 Sep 2032 Jun months 1 month 9 months 11 months 9 months Launch Ariane-5 Jupiter orbit insertion Transfer to Callisto Europa.
BEPICOLOMBO MERCURY MISSION. The main questions about Mercury Why Mercury is so dense? What is the geological history of Mercury? What is the structure.
Lecture 3-Building a Detector (cont’d) George K. Parks Space Sciences Laboratory UC Berkeley, Berkeley, CA.
Observation of cosmic gamma-ray bursts and solar flares in the ''RELEC'' experiment on the ''VERNOV'' satellite.
High-energy Electron Spectrum From PPB-BETS Experiment In Antarctica Kenji Yoshida 1, Shoji Torii 2 on behalf of the PPB-BETS collaboration 1 Shibaura.
An electron/positron energy monitor based on synchrotron radiation. I.Meshkov, T. Mamedov, E. Syresin, An electron/positron energy monitor based on synchrotron.
PoGO_collimator_ ppt1 Study of PoGO background dependence on the collimator material/slow scintillator threshold April 21, 2004 Tsunefumi Mizuno.
PoGO_G4_ ppt1 Study of optimized fast scintillator length for the astronomical hard X- ray/soft gamma-ray polarimeter PoGO November 1, 2004 Tsunefumi.
© The Aerospace Corporation 2010 Use of Geant4 Simulations to Understand LRO/CRaTER Observations M. D. Looper, J. E. Mazur, J. B. Blake, The Aerospace.
Pedro Brogueira 1, Patrícia Gonçalves 2, Ana Keating 2, Dalmiro Maia 3, Mário Pimenta 2, Bernardo Tomé 2 1 IST, Instituto Superior Técnico, 2 LIP, Laboratório.
The highly miniaturised radiation monitor Edward Mitchell * On behalf of the HMRM collaboration (STFC Rutherford Appleton Laboratory & Imperial College.
Encontro com a Ciência e a Tecnologia em Portugal 4-7 Julho 2010.
Dose Mapping for the SIXS Module and X-ray detector BepiColombo Mission 7 th GEANT4 Space Users’ Workshop August 18 – 20, 2010 Seattle - USA F. García,
Gyeongbok Jo 1, Jongdae Sohn 2, KyeongWook Min 2, Yu Yi 1, Suk-bin Kang 2 1 Chungnam National University 2 Korea Advanced Institute of Science.
by students Rozhkov G.V. Khalikov E.V. scientific adviser Iyudin A.F.
European Space Weather Week - 13
Models for the Simulation of X-Ray Fluorescence and PIXE
The Transition Radiation Detector for the PAMELA Experiment
Radiation hardness tests of GaAs and Si sensors at JINR S. M
Project Structure Advanced Neutron Spectrometer on the International Space Station (ANS-ISS) Mark Christl NASA/MSFC Oct 23, 2015 Honolulu, HI 1 1.
KM2A Electron Detector Optimization
R. Bucˇık , K. Kudela and S. N. Kuznetsov
Test Beam Simulation for ESA BepiColombo Mission
1. Introduction Secondary Heavy charged particle (fragment) production
CRaTER Science Requirements
CRaTER Science Requirements
Recent, undergoing and planned ESA-supported activities concerning development, use and promotion of the Geant4 toolkit E. Daly, R. Nartallo, P. Nieminen.
The Hadrontherapy Geant4 advanced example
esa. int/solar-orbiter/51168-summary/;
HE instrument and in-orbit performance
Presentation transcript:

6 October 2005 Geant4 Workshop, Leuven, Belgium Geant4 Model of SIXS Particle Instrument and Preliminary Simulation Results Lehti, J. (ASRO) Valtonen, E. (ASRO) Vainio, R. (University of Helsinki)

6 October 2005Geant4 Workshop, Leuven, Belgium Outline SIXS particle instrument SIXS particle instrument Geant4 model of SIXS Geant4 model of SIXS Simulations results Simulations results Future plans Future plans

6 October 2005Geant4 Workshop, Leuven, Belgium SIXS Experiment SIXS Experiment Solar Intensity X-ray and particle Spectrometer onboard MPO Scientific objectives: Provide the primary solar radiation spectrum for X-ray fluorescence measurements Study coronal X-ray and energetic particle emission BepiColombo - SIXS BepiColombo mission BepiColombo mission ESA cornerstone mission to Mercury ESA cornerstone mission to Mercury Launch 2012 Launch 2012 Five years’ cruise phase, one year operation at orbit Five years’ cruise phase, one year operation at orbit Double S/C mission: Double S/C mission: Mercury Planetary Orbiter (MPO) Mercury Planetary Orbiter (MPO) three-axis stabilized three-axis stabilized z-axis nadir pointing z-axis nadir pointing 400 x 1500 km orbit 400 x 1500 km orbit Mercury Magnetospheric Orbiter (MMO) Mercury Magnetospheric Orbiter (MMO)

6 October 2005Geant4 Workshop, Leuven, Belgium SIXS Particle Instrument SIXS Particle Instrument SIXS Particle Instrument 2π sr Field-of-View around anti-nadir with Geometric Factor of ~ 0.1 cm2 sr Five GaAs surface detectors around a HgI2 core detector Measures MeV electrons MeV protons ΔE/E ~ 50 % energy channel separation coarse directional resolution 64-s/1-s time resolution

6 October 2005Geant4 Workshop, Leuven, Belgium Geant4 model (1/2) Geometry Geometry Core detector Core detector 4x4x4 mm3 4x4x4 mm3 Mercuric iodide (HgI 2 ) Mercuric iodide (HgI 2 ) Side detectors Side detectors Thickness 50 μm Thickness 50 μm Gallium Arsenide (GaAs) Gallium Arsenide (GaAs) Supporting structure Supporting structure Aluminum Aluminum G4Box solids (16 pcs) G4Box solids (16 pcs) Foils above side detectors Foils above side detectors Thickness 25 μm Thickness 25 μm Beryllium Beryllium Screen capture from VRML browser

6 October 2005Geant4 Workshop, Leuven, Belgium Geant4 model (2/2) Physics Physics LE EM package LE EM package Output Output Ascii file Ascii file CSV CSV Human readable Human readable Easy to read with different analysis software Easy to read with different analysis software Energy losses and incident direction Energy losses and incident direction

6 October 2005Geant4 Workshop, Leuven, Belgium Simulations Electron and proton separation Particle identification is based on ΔE/E method Particle identification is based on ΔE/E method Special case

6 October 2005Geant4 Workshop, Leuven, Belgium Simulations Electron and proton separation Special case: Special case: Particles do not trigger the core detector Particles do not trigger the core detector  Separation is not possible Solution: Solution: Reduce from the detected Reduce from the detected intensity the intensity of the protons which stopped in the side detector Energy Intensity ~1.4 MeV

6 October 2005Geant4 Workshop, Leuven, Belgium Simulations Electron and proton separation electrons protons

6 October 2005Geant4 Workshop, Leuven, Belgium Simulations Energy resolution Isotropic and beam particle sources Isotropic and beam particle sources Beam represents a “perfect” collimation Beam represents a “perfect” collimation Detected energy channels are normalized to unity Detected energy channels are normalized to unity X-, Y-, Z-axes are logarithmic X-, Y-, Z-axes are logarithmic Ideal instrument  line Ideal instrument  line

6 October 2005Geant4 Workshop, Leuven, Belgium Future plans Geometric factor and response function simulations Geometric factor and response function simulations Use the model to improve performance of the instrument Use the model to improve performance of the instrument More detailed geometry implementation More detailed geometry implementation More realistic particle sources, e.g. real intensity spectra, anisotropies More realistic particle sources, e.g. real intensity spectra, anisotropies